Method of measuring the noise level in the presence of a signal

Abstract: A method of measuring the noise level in the presence of a signal (51) at a signal wavelength (λ signal ), comprises the steps of detuning the signal (51) to a second wavelength different from the signal wavelength, determining a difference function (Delta (λ)) corresponding to the difference in noise levels before and after detuning of the signal as a function of wavelength, measuring the noise level (N* (λ signal )) at the signal wavelength (λ signal ), and adding the value of the difference function (Delta) at the signal wavelength (λ signal ) to the noise level (N* (λ signal )) measured in the previous step. The method is particularly suited for measuring the noise level in an optical amplifier.

Description: The invention relates to a method of measuring the noise level in the presence of a signal. Such a method is used, for example, in noise figure measurements of optical amplifiers. BACKGROUND OF THE INVENTION Optical amplifiers are used in optical telecommunications systems to provide compensation of losses incurred within the optical transmission network. A particularly advantageous type of optical amplifier is the erbium-doped fiber amplifier (EDFA). Important parameters for characterizing an erbium-doped fiber amplifier and other optical amplifiers are gain and noise figure. The noise figure is important in comparing the performance of various amplifier designs and for system design. Noise generated in an erbium-doped fiber amplifier will degrade the signal-to-noise ratio at the optoelectronic receiver and thus increase the bit error rate of an optical communications system. One source of noise is incoherent radiation which is generated in the erbium-doped fiber amplifier, called amplified spontaneous emission. While the measurement of the gain is comparatively straightforward, the measurement of noise figure of optical amplifiers encounters practical difficulties. For example, the noise level must be determined at the wavelength (or frequency) of an optical signal, in the presence of the signal. Both signal and noise are usually displayed on an optical spectrum analyzer as a plot of optical intensity versus wavelength. At the wavelength of the signal, the noise and the signal intensities are superimposed so that it is difficult to determine what the actual noise intensity at this wavelength is. A known method of solving the mentioned problem is to use interpolation. According to this method, the noise levels to the left and to the right of the signal (at a smaller and at a greater wavelength) are measured and the noise level at the signal wavelength is determined by interpolation. An improvement of this method is also known, i.e., taking several samples at various distances from the signal wavelength on each side of the signal wavelength and interpolating to the signal wavelength by spline approximation or polynomial fitting. The optical spectrum analyzer used in the characterization of an erbium-doped fiber amplifier is expected to display, in addition to the signal, amplified spontaneous emission (ASE) only. In reality, the spontaneous emission of the source (SSE) is also amplified by the erbium-doped fiber amplifier and adds to the amplified spontaneous emission. One way of eliminating the spontaneous emission of the source is measuring it before the fiber amplifier is inserted, and subtracting (gain times spontaneous emission of the source) from the displayed spontaneous emission. This method is called "amplified spontaneous emission interpolation/subtraction". Another alternative is the polarization extinction method. This method is based on the fact that the amplified spontaneous emission is completely unpolarized whereas the spontaneous emission of the source is either completely polarized or can be polarized using a polarizer. Then a polarization controller/filter is used to extinguish the polarized spontaneous emission of the source so that only the unpolarized amplified spontaneous emission passes (more precisely, one half of it). A problem with this method is that the polarization mode dispersion of the erbium-doped fiber amplifier reduces the amount of suppression of spontaneous emission of the source at wavelengths away from the signal wavelength. The larger the wavelength difference and/or the polarization mode dispersion, the less perfect the suppression. This leads to the - sometimes strong - wavelength dependence of the combined (ASE + Gain times SSE)-signal (a dip at the signal wavelength) on the optical spectrum analyzer when using the polarization extinction method. The known methods of measuring the noise level suffer from limited accuracy, particularly because sometimes the noise level exhibits a strong curvature near the signal wavelength. In the polarization extinction technique, the noise level may have a strong curvature near the signal wavelength as this is an inherent property of this technique. It is apparent that such a curvature makes it difficult to determine the actual noise intensity at the signal wavelength. The polarization extinction technique and some other methods for determining noise figure in optical amplifiers are described in D. Baney, C. Hentschel, J. Dupre: "Optical Fiber Amplifiers", Lightwave Symposium 1993. From Patent Abstracts of Japan, Vol.17, No.509 (P-1612), 13 September 1993, a method for measuring the noise level in the presence of a signal in a fiber-optic amplifier is known. In this publication, the following features are disclosed in combination: measuring, at several wavelengths, the noise levels of an original curve representing the optical intensity variation; determining a difference function , wherein the value of the difference function at the signal wavelength is determined by interpolation; adding the value of the difference function at the signal wavelength to the noise level. SUMMARY OF THE INVENTION It is thus an object of the invention to provide a method of measuring the noise level in the presence of a signal which has a higher accuracy. According to the invention, these objects are solved by a method as defined in claim 1. According to an underlying principle of the invention, the signal wavelength is detuned, using for example, a tunable laser source, thereby giving access to the waveshape of the noise at the signal wavelength. The absolute noise level is likely to change as a consequence of detuning. However, this effect can be corrected by curve fitting between the original noise curve and the detuned noise curve. In an embodiment of the invention, the noise levels are measured with an optical spectrum analyzer at a plurality of wavelengths before and after detuning and a difference function is derived therefrom describing the difference in noise levels before and after detuning. From the measurement of the noise level, after detuning, at the original signal wavelength and the interpolated value of the difference function at this wavelength, a corrected noise level at the original signal wavelength is determined. Another advantage of the invention consists in the following: For amplifiers with large polarization mode dispersion, the classical polarization extinction method is not perfectly suited to determine the lowest point of the above mentioned dip displayed on the optical spectrum analyzer. With the method according to the invention, the dip is displayed well (the bottom of the dip represents the point where the spontaneous emission of the source is most strongly suppressed). BRIEF DESCRIPTION OF THE DRAWINGS Subsequently, the invention is explained in more detail with reference to the drawings. Figure 1 shows an embodiment of an apparatus for performing the invention. Figure 2 shows two optical signal curves for illustrating the principle of the invention. DETAILED DESCRIPTION OF THE EMBODIMENTS Figure 1 shows an apparatus for measuring the noise level in an erbium-doped fiber amplifier 10. The amplifier 10 is connected via optical fibers 35 and 36 to an amplifier test set 11. The connection of the fibers 35 and 36 with the amplifier 10 on the one hand and the test set 11 on the other hand is accomplished by means of optical connectors 40, 41, 42, 43. The amplifier test set 11 is connected with an optical fiber 20 to the output of a tunable laser source 14. The tunable laser source 14 provides a coherent light beam the wavelength of which can be adjusted to desired value. An example of such a tunable laser source is the Hewlett-Packard Model No. HP 8168A Tunable Laser Source. The amplifier test set 11 comprises a first optical coupler 15 which directs a certain fraction of the laser light entering the test set 11 to a power meter 22. The branched off laser light is transmitted to the power meter 22 via an optical fiber 21. The test set 11 further comprises a second optical coupler 16 which directs a certain fraction of the laser light which has been transmitted through the first coupler 15 and then through the erbium-doped fiber amplifier 10 to an output terminal 23. For measuring the gain of the erbium-doped fiber amplifier 10, the output terminal 23 is connected to a power meter. The power meter 22, for example, can be used for this purpose. By comparing the optical intensities branched off from the first coupler 15 and from the second coupler 16, respectively, the amplifier gain is determined. According to a practical example, about 1% of the optical intensity incident on the first coupler 15 and about 95% of the optical intensity incident on the second coupler 16 are branched off. The amplifier test set 11 further comprises a polarization controller/filter 12 which partly suppresses the signal and the spontaneous emission from the tunable laser source. As outlined above, the polarization controller/filter is supposed to suppress the spontaneous emission of the source. It will also suppress the signal, because the spontaneous emission of the source has the same state of polarization as the signal. However, the suppression of the signal is not strong enough to be able to measure directly at the signal wavelength. The optical output signal from the polarization controller/filter 12 is transmitted via an optical fiber 24 to an optical spectrum analyzer 13. The optical spectrum analyzer provides a display of light intensity versus wavelength (or frequency). In a practical example, the optical spectrum analyzer is a Hewlett-Packard Model No. HP 71450A Optical Spectrum Analyzer. Instead of passing through the polarization controller/filter 12, the optical signal from the amplifier 10 can directly be transmitted to the optical spectrum analyzer 13. For this purpose, a switching means 17,18 is provided which allows to bypass the polarization controller/filter 12 via an optical transmission line 19. In the following, the individual method steps for measuring the noise level will be described with reference to Figure 2. Figure 2 is a display of curves on the optical spectrum analyzer 13. The horizontal axis is the wavelength of the optical signal, and the vertical axis is the intensity. The upper curve 50 comprises a signal peak 51 at the wavelength λ signal . The noise level at the wavelength λ signal is to be determined. According to a first step of the invention, several noise samples of the curve 50 at predefined wavelengths are measured. These noise samples are labelled with reference numerals 60a, 61a, 62a, 64a, 65a, 66a. In the second step, the entire curve 50 with the signal peak 51 is detuned by a certain wavelength. The detuning is accomplished by changing the wavelength of the output signal of the tunable laser source 14 correspondingly. In a practical example, the signal is detuned by about 1-2 nanometers. The resulting curve on the optical spectrum analyzer 13 is the curve 52 with the signal peak 53. This curve is shifted relative to the original curve 50 with the signal peak 51 by a certain wavelength interval. In the next step, the noise samples on the detuned curve 52 are measured at the same wavelengths as the noise samples of the original curve 50. The noise samples of the detuned curve are labelled with 60b, 61b, 62b, 64b, 65b, 66b. Furthermore, the noise sample 63 at the wavelength λ signal of the original signal peak 51 is measured. The numerical value of the noise sample 63 will be denoted as N* (λ signal ). In the next step, the difference function Delta (λ) is determined. This difference function corresponds to the numerical difference between the noise samples taken at the original curve 50 and those taken at the detuned curve 52 at the same wavelengths, respectively, as a function of the wavelength. Then, the value of the function Delta (λ) is determined at the wavelength λ signal of the original signal peak 51. This is done either by interpolation or by spline approximation or, according to a preferred embodiment, by polynomial fitting. Finally, the correct noise level N (λ signal ) at the wavelength λ signal is determined by adding the value of the difference function at the wavelength λ signal to the value of the noise sample 63: N (λ signal ) = Delta (λ signal ) + N* (λ signal ) . The above described process can be automated, i.e., the measurement of the noise samples at the original and at the detuned curve as well as the necessary calculations are performed automatically under the control of a computer. The described method ensures a much improved accuracy in comparison with the prior art methods based on interpolation. The improvement in accuracy depends on the amount of spontaneous emission of the source, on the polarization mode dispersion of the fiber amplifier, and on the degree of saturation. According to a practical example, improvements on the order of 0.1 to 0.2 dB are possible. The method of the invention can also be used in conjunction with the amplified spontaneous emission (ASE) interpolation/subtraction method, because strong curvature of the wavelength dependence of the ASE is a typical problem caused by the physics of erbium-doped fiber amplifiers. ASE interpolation/subtraction does not need a polarization controller/filter. Even though the method of the invention is particularly suited for noise measurements in optical amplifiers, it is understood that it is not limited to this area, but that it can also be used in other applications wherein noise is to be measured in the presence of a signal.

Claims: A method of measuring the noise level in the presence of a signal (51) at a signal wavelength (λ signal ), comprising the steps of: a) measuring, at several wavelengths, the noise levels (60a, 61a, 62a, 64a, 65a, 66a) of an original curve (50) representing the optical intensity variation, b) detuning the signal (51) to a second wavelength different from the signal wavelength, c) measuring, at several wavelengths, the noise levels (60b, 61b, 62b, 64b, 65b, 66b) of the curve (52) representing the optical intensity variation after detuning, including the noise level (N*(λ signal )) at the signal wavelength (λ signal ), d) determining a difference function (Delta (λ)) corresponding to the numerical difference between the noise samples taken at the original curve (50) and those taken at the detuned curve (52) at the same wavelengths, respectively, as a function of the wavelength, wherein the value of the difference function (Delta) at the signal wavelength (λ signal ) is determined by interpolation or by approximation or by polynomial fitting, and e) adding the value of the difference function (Delta) at the signal wavelength (λ signal ) to the noise level (N*(λ signal )) at the signal wavelength (λ signal ) measured in step c). A method as in claim 1 for measuring the noise level in an optical amplifier, for example an erbium-doped fiber amplifier.

Inventors: HENTSCHEL CHRISTIAN, LECKEL EDGAR, MUELLER EMMERICH, RUECK CLEMENS, HENTSCHEL, CHRISTIAN, LECKEL, EDGAR, MUELLER, EMMERICH, RUECK, CLEMENS, Müller, Emmerich, Rück, Clemens
Applicants: HEWLETT PACKARD GMBH, HEWLETT-PACKARD GMBH
Application year: 1994
Main classification: H04B10
IPC codes: H01S3, G02F1, H04B10, G01M11, G01J3